5 papers
Statistics of Gas Density, Velocity, and Magnetic Fields in Cool-Core Galaxy Clusters
Yue Hu, Alex Lazarian, G. Brunetti +1
Understanding turbulence within the Intracluster Medium (ICM) of galaxy clusters is pivotal for comprehending their evolution and dynamics. Employing 3D magnetohydrodynamic (MHD) s…
Machine Learning Approach for Estimating Magnetic Field Strength in Galaxy Clusters from Synchrotron Emission
Jiyao Zhang, Yue Hu, A. Lazarian
Magnetic fields play a crucial role in various astrophysical processes within the intracluster medium, including heat conduction, cosmic ray acceleration, and the generation of syn…
Origin of the Multi-Phase Interstellar Medium: the Effects of Turbulence and Magnetic Field
Yue Hu
The interstellar medium (ISM) consists of a multiphase gas, including the warm neutral medium (WNM), the unstable neutral medium (UNM), and the cold neutral medium (CNM). While sig…
Estimate Sonic Mach Number in the Interstellar Medium with Convolutional Neural Network
Tyler Schmaltz, Yue Hu, Alex Lazarian
Understanding the role of turbulence in shaping the interstellar medium (ISM) is crucial for studying star formation, molecular cloud evolution, and cosmic ray propagation. Central…
Probing Three-Dimensional Magnetic Fields: IV -- Synchrotron Polarization Derivative and Vision Transformer
Yue Hu, Alex Lazarian
Measuring the 3D spatial distribution of magnetic fields in the interstellar medium and the intracluster medium is crucial yet challenging. The probing of 3D magnetic field's 3D di…